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The latest results from CAST and the IAXO project
The CAST experiment has been the most sensitive helioscope so far. It has extended its sensitivity to the upper bounds of axion masses allowed by cosmology, entering well into the QCD-axion band. The preliminary analysis of the data taken with sensitivity to axion masses of the range 0.64 eV to 1.17...
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Lenguaje: | eng |
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2014
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Acceso en línea: | https://dx.doi.org/10.22323/1.180.0394 http://cds.cern.ch/record/2003074 |
_version_ | 1780946168376721408 |
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author | Dafni, Theopisti |
author_facet | Dafni, Theopisti |
author_sort | Dafni, Theopisti |
collection | CERN |
description | The CAST experiment has been the most sensitive helioscope so far. It has extended its sensitivity to the upper bounds of axion masses allowed by cosmology, entering well into the QCD-axion band. The preliminary analysis of the data taken with sensitivity to axion masses of the range 0.64 eV to 1.17 eV show no excess of signal above background and the coupling constant is restricted to g a g < 3 : 3 10 10 GeV 1 . While CAST continues with the aim to improve its results in the vacuum phase, IAXO is the new project proposed to build a dedicated magnet for axion searches that will supersede CAST’s sensitivity by one order of magnitude in g a g . |
id | oai-inspirehep.net-1290753 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2014 |
record_format | invenio |
spelling | oai-inspirehep.net-12907532019-09-30T06:29:59Zdoi:10.22323/1.180.0394http://cds.cern.ch/record/2003074engDafni, TheopistiThe latest results from CAST and the IAXO projectAstrophysics and AstronomyThe CAST experiment has been the most sensitive helioscope so far. It has extended its sensitivity to the upper bounds of axion masses allowed by cosmology, entering well into the QCD-axion band. The preliminary analysis of the data taken with sensitivity to axion masses of the range 0.64 eV to 1.17 eV show no excess of signal above background and the coupling constant is restricted to g a g < 3 : 3 10 10 GeV 1 . While CAST continues with the aim to improve its results in the vacuum phase, IAXO is the new project proposed to build a dedicated magnet for axion searches that will supersede CAST’s sensitivity by one order of magnitude in g a g .oai:inspirehep.net:12907532014 |
spellingShingle | Astrophysics and Astronomy Dafni, Theopisti The latest results from CAST and the IAXO project |
title | The latest results from CAST and the IAXO project |
title_full | The latest results from CAST and the IAXO project |
title_fullStr | The latest results from CAST and the IAXO project |
title_full_unstemmed | The latest results from CAST and the IAXO project |
title_short | The latest results from CAST and the IAXO project |
title_sort | latest results from cast and the iaxo project |
topic | Astrophysics and Astronomy |
url | https://dx.doi.org/10.22323/1.180.0394 http://cds.cern.ch/record/2003074 |
work_keys_str_mv | AT dafnitheopisti thelatestresultsfromcastandtheiaxoproject AT dafnitheopisti latestresultsfromcastandtheiaxoproject |